Brun's constant
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In 1919 Viggo Brun showed that the sum of the reciprocals of the twin primes (pairs of prime numbers which differ by 2) converges to a mathematical constant now called Brun's constant for twin primes and usually denoted by B2 (sequence A065421 in OEIS):
Brun's sieve was refined by J.B. Rosser, G. Ricci and others. By calculating the twin primes up to 1014 (and discovering the infamous Pentium FDIV bug along the way), Thomas R. Nicely heuristically estimated Brun's constant to be 1.902160578. The best estimate to date was given by Pascal Sebah and Patrick Demichel in 2002, using all twin primes up to 1016:
While 1.9 < B2 is shown, no real number N is known such that B2 < N. There is also a Brun's constant for prime quadruplets. A prime quadruplet is a pair of two twin prime pairs, separated by a distance of 4 (the smallest possible distance). The first prime quadruplets are (5, 7, 11, 13), (11, 13, 17, 19), (101, 103, 107, 109). Brun's constant for prime quadruplets, denoted by B4, is the sum of the reciprocals of all prime quadruplets:
This constant should not be confused with the Brun's constant for cousin primes, prime pairs of the form (p, p + 4), which is also written as B4. Wolf derived an estimate for the Brun-type sums Bn of 4/n. This gives the estimate for Bn of 2, about 5% higher than the true value. See alsoExternal links
de:Brunsche Konstante es:Constante de Brun fr:Constante de Brun it:Costante di Brun he:קבוע ברון lmo:Custanta da Brun hu:Brun-konstans nl:Constante van Brun ja:ブルン定数 pl:Stałe Bruna pt:Constante de Brun |


